Please use this identifier to cite or link to this item: http://nopr.niscpr.res.in/handle/123456789/38910
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dc.contributor.authorMurthy, A Satyanarayana-
dc.contributor.authorRao, M G Seshagiri-
dc.contributor.authorSharm, G S-
dc.date.accessioned2016-12-20T05:48:22Z-
dc.date.available2016-12-20T05:48:22Z-
dc.date.issued1982-03-
dc.identifier.issn0975-1033 (Online); 0379-5136 (Print)-
dc.identifier.urihttp://nopr.niscair.res.in/handle/123456789/38910-
dc.description1-6en_US
dc.description.abstractCirculation pattern in the Arabian Sea is derived from computation of acceleration potential at 2 isanosteric surfaces (400 and 200 cl/t) using oceanographic data obtained during the International Indian Ocean Expedition. As the current structure in the upper layers of the Arabian Sea varies from season to season, the study is limited to the southwest monsoon, when the surface circulation in the North Indian Ocean differs very much from the other 2 major oceans. Maps showing the distribution of acceleration potential at 400 and 200 cl/t surfaces are presented. Distribution of the thickness of the layer between 10 cl/t above and 10 cl/t below each surface is also presented in order to gain quantitative information about the water volume, water flux and stability according to characteristics.en_US
dc.language.isoen_USen_US
dc.publisherNISCAIR-CSIR, Indiaen_US
dc.rights CC Attribution-Noncommercial-No Derivative Works 2.5 Indiaen_US
dc.sourceIJMS Vol.11(1) [March 1982]en_US
dc.titleCurrent structure in the upper layers of the Arabian Sea during southwest monsoonen_US
dc.typeArticleen_US
Appears in Collections:IJMS Vol.11(1) [March 1982]

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